FSR 0167
(MWSC 3244; FoF 162)
0.94
UTI
1.0
CN
1.0
Cdens
1.0
CC3
0.86
Clit
1.0
Cdup
Radius (P>50% members)
8.9 [arcmin]
- CN 1.0 Very rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.86 Well-studied
- Cdup 1.0 Unique
Overview
FSR 0167 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is well-studied in the literature.
Relatively close
High extinction
Massive
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 301.224 | 27.069 | 0.532 | 0.076 | -1.797 | 5.923 |
| Zhang et al. | 2024 | 301.249 | 27.08 | â | â | â | â |
| Hunt & Reffert | 2024 | 301.249 | 27.08 | 0.537 | 0.082 | -1.789 | 27.809 |
| Cavallo et al. | 2024 | 301.219 | 27.074 | 0.535 | â | â | â |
| Hunt & Reffert | 2023 | 301.249 | 27.08 | 0.537 | 0.082 | -1.789 | 27.809 |
| Just et al. | 2023 | 301.209 | 27.091 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 301.218 | 27.057 | 0.533 | 0.102 | -1.83 | â |
| Cantat-Gaudin & Anders | 2020 | 301.218 | 27.057 | 0.533 | 0.102 | -1.83 | â |
| Liu & Pang | 2019 | 301.226 | 27.072 | 0.517 | 0.1 | -1.778 | â |
| Soubiran et al. | 2018 | 301.218 | 27.057 | â | â | â | 1.77 |
| Bica et al. | 2019 | 301.212 | 27.067 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 301.218 | 27.057 | 0.533 | 0.102 | -1.83 | â |
| Kharchenko et al. | 2016 | 301.209 | 27.091 | â | â | â | â |
| Dias et al. | 2014 | 301.208 | 27.071 | â | 0.56 | 3.22 | â |
| Kharchenko et al. | 2013 | 301.215 | 27.093 | â | -0.27 | -4.75 | â |
| Froebrich et al. | 2007 | 301.208 | 27.071 | â | â | â | â |
| Dias et al. | 2002 | 301.208 | 27.071 | â | 0.56 | 3.22 | â |
đĄ Note: The UCC values are estimated from its identified members.
| Reference | Year | Dist [kpc] | Av [mag] | DAv [mag] | Age [Myr] | [Fe/H] [dex] | Mass [Msun] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Zhang et al. | 2024 | â | â | â | â | -0.259* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 6333* | â | â |
| Cavallo et al. | 2024 | 2.09 | 3.88 | â | 138 | 0.480 | â | â | â |
| Hunt & Reffert | 2023 | 1.76 | 3.89 | 2.67 | 175 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 158 | â | 54 | â | â |
| Cantat-Gaudin et al. | 2020 | 1.77 | 2.52 | â | 776 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.78 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 576 | 0.250 | â | â | â |
| Soubiran et al. | 2018 | 1.78 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.78 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 1.99 | 3.87 | â | 158 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.99 | 3.87 | â | 158 | â | â | â | â |
| Dias et al. | 2002 | 1.99 | 3.87 | â | 158 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.